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NSR database version of May 19, 2024.

Search: Author = A.Sweet

Found 4 matches.

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2024CO05      Phys.Rev.Lett. 132, 152503 (2024)

I.Cox, Z.Y.Xu, R.Grzywacz, W.-J.Ong, B.C.Rasco, N.Kitamura, D.Hoskins, S.Neupane, T.J.Ruland, J.M.Allmond, T.T.King, R.S.Lubna, K.P.Rykaczewski, H.Schatz, B.M.Sherrill, O.B.Tarasov, A.D.Ayangeakaa, H.C.Berg, D.L.Bleuel, G.Cerizza, J.Christie, A.Chester, J.Davis, C.Dembski, A.A.Doetsch, J.G.Duarte, A.Estrade, A.Fijalkowska, T.J.Gray, E.C.Good, K.Haak, S.Hanai, J.T.Harke, C.Harris, K.Hermansen, D.E.M.Hoff, R.Jain, M.Karny, K.Kolos, A.Laminack, S.N.Liddick, B.Longfellow, S.Lyons, M.Madurga, M.J.Mogannam, A.Nowicki, T.H.Ogunbeku, G.Owens-Fryar, M.M.Rajabali, A.L.Richard, E.K.Ronning, G.E.Rose, K.Siegl, M.Singh, A.Spyrou, A.Sweet, A.Tsantiri, W.B.Walters, R.Yokoyama

Proton Shell Gaps in N=28 Nuclei from the First Complete Spectroscopy Study with FRIB Decay Station Initiator

RADIOACTIVITY 45Cl(β-) [from 9Be(82Se, X), E=165 MeV/nucleon]; measured decay products, Eγ, Iγ, Eβ, Iβ; deduced β-decay strength distribution, the transitioning of neutrons into protons excited across the Z=20 shell gap. Comparison with shell model calculations using SDPF-MU interaction. The Facility for Rare Isotope Beams (FRIB) with the FRIB Decay Station Initiator.

doi: 10.1103/PhysRevLett.132.152503
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2024SP04      Phys.Rev.Lett. 132, 202701 (2024)

A.Spyrou, D.Mucher, P.A.Denissenkov, F.Herwig, E.C.Good, G.Balk, H.C.Berg, D.L.Bleuel, J.A.Clark, C.Dembski, P.A.DeYoung, B.Greaves, M.Guttormsen, C.Harris, A.C.Larsen, S.N.Liddick, S.Lyons, M.Markova, M.J.Mogannam, S.Nikas, J.Owens-Fryar, A.Palmisano-Kyle, G.Perdikakis, F.Pogliano, M.Quintieri, A.L.Richard, D.Santiago-Gonzalez, G.Savard, M.K.Smith, A.Sweet, A.Tsantiri, M.Wiedeking

First Study of the 139Ba(n, γ)140Ba Reaction to Constrain the Conditions for the Astrophysical i Process

RADIOACTIVITY 140Cs(β-); measured decay products, Eγ, Iγ; deduced γ-ray energies, γ-ray strength functions, nuclear level density, astrophysical reaction rates. Comparison with TALYS calculations. β-Oslo method, the CARIBU facility at Argonne National Laboratory.

doi: 10.1103/PhysRevLett.132.202701
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2020LA18      J.Instrum. 15, P11020 (2020)

T.A.Laplace, B.L.Goldblum, J.E.Bevins, D.L.Bleuel, E.Bourret, J.A.Brown, E.J.Callaghan, J.S.Carlson, P.L.Feng, G.Gabella, K.P.Harrig, J.J.Manfredi, C.Moore, F.Moretti, M.Shinner, A.Sweet, Z.W.Sweger

Comparative scintillation performance of EJ-309, EJ-276, and a novel organic glass

doi: 10.1088/1748-0221/15/11/P11020
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2019HU07      Phys.Rev. C 99, 024310 (2019)

A.M.Hurst, A.Sweet, B.L.Goldblum, R.B.Firestone, M.S.Basunia, L.A.Bernstein, Zs.Revay, L.Szentmiklosi, T.Belgya, J.E.Escher, I.Harsanyi, M.Krticka, B.W.Sleaford, J.Vujic

Radiative-capture cross sections for the 139La (n, γ) reaction using thermal neutrons and structural properties of 140La

NUCLEAR REACTIONS 139La(n, γ), E=thermal and cold; measured Eγ, Iγ, at the Prompt Gamma Activation Analysis facility of Budapest Research Reactor. 140La; deduced levels, J, π, S(n) for 140La, partial γ-ray production σ(γ) relative to those for 35Cl(n, γ), total radiative thermal neutron capture σ. Monte Carlo statistical-decay code DICEBOX calculations. Comparison with previous experimental data in the ENSDF database and other literature.

doi: 10.1103/PhysRevC.99.024310
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset31795.

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